Kinman, T. D.T. D.KinmanBRAGAGLIA, AngelaAngelaBRAGAGLIACacciari, C.C.CacciariBUZZONI, AlbertoAlbertoBUZZONISPAGNA, AlessandroAlessandroSPAGNA2024-01-302024-01-3020040037-8720http://hdl.handle.net/20.500.12386/34659New GSC-II proper motions and radial velocities of RR Lyrae and Blue Horizontal Branch stars near the North Galactic Pole are used to show that the Galactic Halo 5 kpc above the Plane has a significantly retrograde galactic rotation. Streaming motions cannot be excluded.STAMPAenThe Vertical Structure of the Halo RotationArticleFIS/05 - ASTRONOMIA E ASTROFISICA